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Out of the Void Poster by Bebops
Thursday, September 17, 2015
Zazzle Favor Bags from Bebops: Rhode Island Red Hen Chicken Favor Bag
Wednesday, September 16, 2015
Carina Nebula, Argo Navis Wristwatch
A gorgeous something for Valentine's day to express your love and featuring a cute animal. Click to see, personalize and buy.
tagged with: hrwaulb, astronomy, carina nebula, argos navis constellation, carina the keel, star formation, carnebngcttst, ngc 3372, star galaxies, hrbstslr carnebngcttst, outer space, gas clouds
Galaxies, Stars and Nebulae series: Hubble's view of the Carina Nebula shows star birth in a new level of detail. The fantasy-like landscape of the nebula is sculpted by the action of outflowing winds and scorching ultraviolet radiation from the monster stars that inhabit this inferno. In the process, these stars are shredding the surrounding material that is the last vestige of the giant cloud from which the stars were born. The immense nebula is an estimated 7,500 light-years away in the southern constellation Carina the Keel (of the old southern constellation Argo Navis, the ship of Jason and the Argonauts, from Greek mythology).
The original image is a mosaic of the Carina Nebula assembled from 48 frames taken with Hubble Space Telescope's Advanced Camera for Surveys. The Hubble images were taken in the light of ionized hydrogen. Colour information was added with data taken at the Cerro Tololo Inter-American Observatory in Chile. Red corresponds to sulfur, green to hydrogen, and blue to oxygen emission.
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image code: carnebngcttst
Image credit: Hubble Space Telescope; colour data from the Cerro Tololo Inter-American Observatory, Chile
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Zazzle Necklace from Bebops: Rhode Island Red Hen Chicken Necklace
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Tuesday, September 15, 2015
Monogram Cats Eye Nebula, Eye of God outer space Trifold Wallet
A gorgeous something for Valentine's day to express your love and featuring a cute animal. Click to see, personalize and buy.
tagged with: nebulae, hubble chandra images, cats eye nebula, dying star, red giant evolution, outer space, galaxy stars, deep space astronomy, eye of god, hrbstslr tcenebnch, stellar evolution, nasa
Galaxies, Stars and Nebulae series A gorgeous design featuring a composite image of the Cat's Eye nebula from NASA's Chandra X-ray Observatory and the Hubble Space Telescope.
This famous nebula represents a phase of stellar evolution after a star like our Sun runs out of fuel. In this phase, a star becomes an expanding red giant and sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures.
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image code: tcenebnch
Image credit: NASA/Chandra www.nasa.gov
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Zazzle Spiral Photo Notebook from Bebops: Rhode Island Red Hen Chicken...
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Zazzle Button from Bebops: Rhode Island Red Hen Chicken Button
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Monday, September 14, 2015
Starry Wingtip of Small Magellanic Cloud Double-Sided Standard Business Cards (Pack Of 100)
A gorgeous something for Valentine's day to express your love and featuring a cute animal. Click to see, personalize and buy.
tagged with: small magellanic cloud, star galaxies, starry, outer space picture, deep space image, galactic, universe exploration, deep space astronomy, interstellar, wismcg genbct1a hrbstslr
Galaxies, Stars and Nebulae series The tip of the "wing" of the Small Magellanic Cloud galaxy is dazzling in this new view from NASA's Great Observatories. The Small Magellanic Cloud, or SMC, is a small galaxy about 200,000 light-years way that orbits our own Milky Way spiral galaxy.
The colors represent wavelengths of light across a broad spectrum. X-rays from NASA's Chandra X-ray Observatory are shown in purple; visible-light from NASA's Hubble Space Telescope is colored red, green and blue; and infrared observations from NASA's Spitzer Space Telescope are also represented in red.
The spiral galaxy seen in the lower corner is actually behind this nebula. Other distant galaxies located hundreds of millions of light-years or more away can be seen sprinkled around the edge of the image.
The SMC is one of the Milky Way's closest galactic neighbors. Even though it is a small, or so-called dwarf galaxy, the SMC is so bright that it is visible to the unaided eye from the Southern Hemisphere and near the equator. Many navigators, including Ferdinand Magellan who lends his name to the SMC, used it to help find their way across the oceans.
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image code: wismcg
Image credit: NASA/CXC/JPL-Caltech/STScI
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Zazzle Button from ValeriesGallery: Cat Piper Button
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Sunday, September 13, 2015
Monogram Barred Spiral Galaxy NGC 1672 Case For iPad Air
A gorgeous something for Valentine's day to express your love and featuring a cute animal. Click to see, personalize and buy.
tagged with: monogram initials, star galaxies, deep space astronomy, barred spiral galaxy, starry space picture, galactic arms, supermassive black hole, dust lanes, star forming galaxy, hrbstslr bsgsst
Galaxies, Stars and Nebulae series This NASA Hubble Space Telescope view of the nearby barred spiral galaxy NGC 1672 unveils details in the galaxy's star-forming clouds and dark bands of interstellar dust.
One of the most striking features is the dust lanes that extend away from the nucleus and follow the inner edges of the galaxy's spiral arms. Clusters of hot young blue stars form along the spiral arms and ionize surrounding clouds of hydrogen gas that glow red. Delicate curtains of dust partially obscure and redden the light of the stars behind them by scattering blue light.
Galaxies lying behind NGC 1672 give the illusion they are embedded in the foreground galaxy, even though they are really much farther away. They also appear reddened as they shine through NGC 1672's dust. A few bright foreground stars inside our own Milky Way Galaxy appear in the image as bright and diamond-like objects.
As a prototypical barred spiral galaxy, NGC 1672 differs from normal spiral galaxies, in that the arms do not twist all the way into the center. Instead, they are attached to the two ends of a straight bar of stars enclosing the nucleus. Viewed nearly face on, NGC 1672 shows intense star formation regions especially off in the ends of its central bar.
Astronomers believe that barred spirals have a unique mechanism that channels gas from the disk inward towards the nucleus. This allows the bar portion of the galaxy to serve as an area of new star generation.
NGC 1672 is also classified as a Seyfert galaxy. Seyferts are a subset of galaxies with active nuclei. The energy output of these nuclei can sometimes outshine their host galaxies. This activity is powered by accretion onto supermassive black holes.
NGC 1672 is more than 60 million light-years away in the direction of the southern constellation Dorado. These observations of NGC 1672 were taken with Hubble's Advanced Camera for Surveys in August of 2005. The composite image was made by using filters that isolate light from the blue, green, and infrared portions of the spectrum, as well as emission from ionized hydrogen.
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image code: bsgsst
Image credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration
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